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Galactic Soft X-Ray Halo Revealed with Suzaku
https://jaxa.repo.nii.ac.jp/records/4987
https://jaxa.repo.nii.ac.jp/records/4987105ae345-9119-446e-b25b-33a4b8239e55
名前 / ファイル | ライセンス | アクション |
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64574055.pdf (349.3 kB)
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Item type | 会議発表論文 / Conference Paper(1) | |||||
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公開日 | 2015-03-26 | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | Galactic Soft X-Ray Halo Revealed with Suzaku | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | Galaxy: disk - Galaxy: halo - X-rays: diffuse background - X-rays: ISM | |||||
資源タイプ | ||||||
資源タイプ識別子 | http://purl.org/coar/resource_type/c_5794 | |||||
資源タイプ | conference paper | |||||
著者 |
山崎, 典子
× 山崎, 典子× 満田, 和久× 竹井, 洋× 吉野, 友崇× 萩原, 利士成× 藤本, 龍一× Yamasaki, Noriko Y× Mitsuda, Kazuhisa× Takei, Yoh× Yoshino, Tomotaka× Hagihara, Toshishige× Fujimoto, Ryuichi× Bauer, Michael× McCammon, Dan× Wang, Q. Daniel× Yao, Yangsen |
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著者所属 | ||||||
宇宙航空研究開発機構宇宙科学研究本部 | ||||||
著者所属 | ||||||
宇宙航空研究開発機構宇宙科学研究本部 | ||||||
著者所属 | ||||||
宇宙航空研究開発機構宇宙科学研究本部 | ||||||
著者所属 | ||||||
宇宙航空研究開発機構宇宙科学研究本部 | ||||||
著者所属 | ||||||
宇宙航空研究開発機構宇宙科学研究本部 | ||||||
著者所属 | ||||||
金沢大学理学部物理学科 | ||||||
著者所属(英) | ||||||
en | ||||||
Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (ISAS)(JAXA) | ||||||
著者所属(英) | ||||||
en | ||||||
Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (ISAS)(JAXA) | ||||||
著者所属(英) | ||||||
en | ||||||
Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (ISAS)(JAXA) | ||||||
著者所属(英) | ||||||
en | ||||||
Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (ISAS)(JAXA) | ||||||
著者所属(英) | ||||||
en | ||||||
Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (ISAS)(JAXA) | ||||||
著者所属(英) | ||||||
en | ||||||
Department of Physics, Kanazawa University | ||||||
著者所属(英) | ||||||
en | ||||||
Max-Planck-Institut f¨ur extraterrestrische Physik | ||||||
著者所属(英) | ||||||
en | ||||||
Department of Physics, University of Wisconsin | ||||||
著者所属(英) | ||||||
en | ||||||
Department of Astronomy, University of Massachusetts Amherst | ||||||
著者所属(英) | ||||||
en | ||||||
University of Colorado | ||||||
出版者 | ||||||
出版者 | 宇宙航空研究開発機構 | |||||
出版者(英) | ||||||
出版者 | Japan Aerospace Exploration Agency (JAXA) | |||||
書誌情報 |
宇宙航空研究開発機構特別資料: en : JAXA Special Publication: The Energetic Cosmos; from Suzaku to ASTRO-H 巻 JAXA-SP-09-008E, p. 150-153, 発行日 2010-02-26 |
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会議概要(会議名, 開催地, 会期, 主催者等)(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | The 3rd Suzaku international Conference "Energetic Cosmos : from Suzaku to ASTRO-H" (June 29-July 2, 2009. Grand Park Otaru Hotel), Otaru, Hokkaido Japan | |||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Spectroscopic study of Oxygen emission/absorption lines is a new tool to investigate the nature of the soft X-ray background. Base on the Suzaku observations of 14 fields, two components of the Oxygen line emission are discovered. One component emits within approximately 300 pc of our neighborhood and most plausible origin is the solar wind charge exchange with local interstellar materials. The other shows an apparent temperature of approximately 0.2 keV with a field-to-field fluctuation of +/- 10 %, while the intensity varies about a factor of 4. By the combination analysis of the emission and the absorption by Oxygens, the size of the hot plasma is an order of kpc. It suggests that there is a hot halo around our Galaxy which is similar to X-ray hot haloes around several spiral galaxies. | |||||
内容記述(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Meeting sponsors: The University of Tokyo, The Institute of Physical and Chemical Research, The Japan Society for the Promotion of Science | |||||
ISSN | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 1349-113X | |||||
書誌レコードID | ||||||
収録物識別子タイプ | NCID | |||||
収録物識別子 | AA11984031 | |||||
資料番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: AA0064574055 | |||||
レポート番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | レポート番号: JAXA-SP-09-008E |